The effect of proton temperature anisotropy on the solar minimum corona and wind
A semiempirical, axisymmetric model of the solar minimum corona is developed by solving the equations for conservation of mass and momentum with prescribed anisotropic temperature distributions. In the high-latitude regions, the proton temperature anisotropy is strong and the associated mirror force...
Guardado en:
| Autores principales: | Vásquez, A.M., Van Ballegooijen, A.A., Raymond, J.C. |
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| Formato: | JOUR |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004637X_v598_n2I_p1361_Vasquez |
| Aporte de: |
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